Hydrodynamics of Black Hole–Accretion Disk Collision

1998 ◽  
Vol 507 (1) ◽  
pp. 131-144 ◽  
Author(s):  
Pavel B. Ivanov ◽  
Igor V. Igumenshchev ◽  
Igor D. Novikov
1999 ◽  
Vol 526 (1) ◽  
pp. 152-177 ◽  
Author(s):  
Chris L. Fryer ◽  
S. E. Woosley ◽  
Dieter H. Hartmann

2015 ◽  
Vol 92 (6) ◽  
Author(s):  
Chinmoy Bhattacharjee ◽  
Rupam Das ◽  
David J. Stark ◽  
S. M. Mahajan

2019 ◽  
Vol 100 (4) ◽  
Author(s):  
T. S. H. Schilbach ◽  
O. L. Caballero ◽  
G. C. McLaughlin

2018 ◽  
Vol 859 (1) ◽  
pp. 28 ◽  
Author(s):  
Qian Qian ◽  
Christian Fendt ◽  
Christos Vourellis

1997 ◽  
Vol 163 ◽  
pp. 53-62
Author(s):  
R. M. Hjellming

AbstractThe superluminal radio jets produced by GRO J1655–40 during a series of X-ray outbursts in 1994 were the first indications of a delayed form of relativistic outflows from black hole accretion disk environments. In this paper we review the relation between the radio jets and changes in the X-ray environment for the 1994 events in GRO J1655–40 and compare this behavior with similar X-ray-radio correlations that have since been found in GRS 1716–249, GRS 1739–278, and the 1996 recurrence of another correlated event in GRO 1655–40. We also discuss newly found radio-X-ray correlations in a galactic X-ray binary, Cyg X–3.


Sign in / Sign up

Export Citation Format

Share Document